Galaxies and Clusters, WFPC GTO Augmentation, Cycle 4

Details Galaxies and Clusters, WFPC GTO Augmentation, Cycle 4 Galaxies and Clusters, WFPC GTO Augmentation, Cycle 4

Jul 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994hst..prop.5741w&link_type=abstract

HST Proposal ID #5741

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Hst Proposal Id #5741 Galaxies &Amp, Clusters

Scientific paper

We propose to observe 10 galaxy nuclei from the original GTO proposal 1118 that otherwise will be lost for lack of time. These 10 include seven of the nearest normal spiral galaxies, from types S0 through Sc. This is the largest sample of late-type spiral nuclei being done with HST that we know of and is essential to the collection of a representative catalog of all galaxy types. The remaining three galaxies include a classic Seyfert galaxy (NGC 4151), a protype emission- line elliptical (NGC 1052), and a well known blue elliptical that is a post-starburst and merger candidate (NGC 1600).

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